sound waves - university of california, san diegokeni.ucsd.edu/f14/lec3.pdf · 2013. 10. 15. ·...
TRANSCRIPT
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Sound Waves
Ken Intriligator’s week 3 lectures, Oct 14, 2013
Ken: “OK,let’s get started..”
Tuesday, October 15, 2013
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Sound = pressure waves(!x, t)displacement fluctuation
satisfies 3d wave equation:s(!x, t) (∇2 −1
v2∂2
∂t2)s("x, t) = 0
∇2f(r) =
1
r
∂2
∂r2(rf(r))
r = spherical, radial coordinate
∇2
=∂2
∂x2+
∂2
∂y2+
∂2
∂z2
Tuesday, October 15, 2013
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3d wave eqn. solutions s(!x, t) = A cos(!k · !x − ωt + φ)“Plane wave”
unit vector point in dir. of wave velocity
!k = kn̂ k =2π
λn̂ =
ω = vk
“Spherical wave” s(r, t) =A
rcos(kr − ωt + φ)
ω = vk
Consider first plane waves, in the x direction:
s(x, t) = A cos(kx − ωt + φ)
Tuesday, October 15, 2013
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Derive the wave eqn.:p(x, t) = gauge pressure ptot = p0 + p
p = −B(dV/V ) B= “bulk modulus,” it’s just like the spring constant k in F = -kx.
F/V = (m/V )a −∂p
∂x= B
∂2s
∂x2= ρ0
∂2s
∂t2
vsound =
√
B
ρ0
Fits with D.A.!
p = −B∂s
∂x
(“Incompressible” fluid has B=infinity)
∂2s
∂x2=
1
v2
∂2s
∂t2
dx
A
Tuesday, October 15, 2013
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Examples
vsound =
√
B
ρ0
Water: ρ0 = 10
3kg/m3B = 2.18 × 10
9Pavsound ≈ 1480m/s
vsound ≈ 344m/sAir: vgas =√
γkT
m
We’ll understand gasses later. For this week, ignoreall parts of the chapter mentioning temperature T.
Ignore thisnow, for later.
Tuesday, October 15, 2013
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Ear’s f (freq) rangesvsound ≈ 344m/s
vsound = λ/T = λf
20Hz ≤ f ≤ 20, 000Hz1.7cm ≤ λ ≤ 17.5m
Humans:
Dogs: 40Hz ≤ f ≤ 60, 000Hz
Cats: 60Hz ≤ f ≤ 80, 000Hz
Bats: 10, 000Hz ≤ f ≤ 200, 000Hz
75Hz ≤ f ≤ 150, 000HzDolphin:
Tuesday, October 15, 2013
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Piano
Tuesday, October 15, 2013
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Pressure Wave eqn.∂2s
∂x2=
1
v2
∂2s
∂t2
∂2p
∂x2=
1
v2∂2p
∂t2
p = −B∂s
∂x·B
∂
∂x
Displacement wave equation:
So get same wave eqn for pressure
s(x, t) = A cos(k(x − vt) + φ0)
p(x, t) = BkA sin(k(x − vt) + φ0)
pmax = BkA = (vρ)(Aω)Larger A (louder) or higher frequencygives bigger p, this can hurt your ears!
Multiply both sides of the s wave eqn. by
(Derived a few slides ago.)
Tuesday, October 15, 2013
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Ouch!s(x, t) = A cos(k(x − vt) + φ0)
p(x, t) = BkA sin(k(x − vt) + φ0)
pmax = BkA = (vρ)(Aω)Larger A (louder) or higher frequencygives bigger p, this can hurt your ears!
Largest gauge pressure before damaging your ears:
pmax ≈ 28Pa v ≈ 343m/s ρair ≈ 1.21kg/m3
(Aω)max ≈ 28/(343)(1.21) ≈ 0.067m/s
e.g. f = 103Hz = ω/2π Amax ≈ 1.1× 10−5mSound wave amplitude, at this frequency, should
be less, or you’ll damage your ears.
Tuesday, October 15, 2013
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Intensity I =
Power
AreaLine on top means “average”, sometimes we also use
these brackets < > to denote averaging.
I =dE
dt=
dK
dt+
dU
dt= 2
dK
dtLike the harmonic oscillator, all oscillatingsystems have average K and U are equal.
dK
dt=
1
2
dm
dt
�∂s
∂t
�2=
1
2ρArea
dx
dt
�∂s
∂t
�2
=1
2ρ(Area)vsoundω
2s2max sin2(kx− ωt+ φ)
s = smax cos(kx− ωt+ φ)
I =1
2ρvsoundω
2s2max
(sin2(∗) = 12)
(For point source, s ~ 1/r)
Ipoint source = Ps/4πr2
(Area).
Tuesday, October 15, 2013
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Intensity & sound levelβ ≡ (10dB) log10(I/10−12W/m2)
I = 10−12W/m2 → β = 0 “What?” Too quiet to hear.
Conversation has beta about 60dB. Loud rock concert is about 110dB. Pain threshold is about 120dB.
Human senses (hearing, seeing, touch, smell, taste) detect intensities I on a log scale. Which is good! Can detect over a large I range, from faint to huge.
Tuesday, October 15, 2013
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Waves in pipes!s=0 at
closed endsp (gauge) =0 at open ends
p = −B∂s
∂x
∂s
∂x|open = 0s|closed = 0
So, the wave eqn. BCs are:
and
(Just like with astring at fixed end.)
(Just like with astring at a free end.)
Tuesday, October 15, 2013
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Pipe wave harmonics
λ = 4L/nodd λ = 2L/nOne end open, one end closed
Both open, or both closed
(Drawingwave’s s
displacement.Pressure is
~ derivative,so opposite.)
Tuesday, October 15, 2013
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s & p in pipes
Tuesday, October 15, 2013
http://www.google.com/imgres?q=wave+in+pipe&client=safari&rls=en&biw=1039&bih=635&tbm=isch&tbnid=4yOfGhJDUL8_xM:&imgrefurl=http://www.acs.psu.edu/drussell/Demos/StandingWaves/StandingWaves.html&docid=rQL8NLCVyxArsM&imgurl=http://www.acs.psu.edu/drussell/Demos/StandingWaves/Opentubeoneend.jpg&w=1600&h=742&ei=VYNZUoyAK4aOigLhvoCABA&zoom=1&ved=1t:3588,r:26,s:0,i:165&iact=rc&page=3&tbnh=153&tbnw=330&start=26&ndsp=16&tx=209&ty=74http://www.google.com/imgres?q=wave+in+pipe&client=safari&rls=en&biw=1039&bih=635&tbm=isch&tbnid=4yOfGhJDUL8_xM:&imgrefurl=http://www.acs.psu.edu/drussell/Demos/StandingWaves/StandingWaves.html&docid=rQL8NLCVyxArsM&imgurl=http://www.acs.psu.edu/drussell/Demos/StandingWaves/Opentubeoneend.jpg&w=1600&h=742&ei=VYNZUoyAK4aOigLhvoCABA&zoom=1&ved=1t:3588,r:26,s:0,i:165&iact=rc&page=3&tbnh=153&tbnw=330&start=26&ndsp=16&tx=209&ty=74http://www.google.com/imgres?q=wave+in+pipe&client=safari&rls=en&biw=1039&bih=635&tbm=isch&tbnid=4yOfGhJDUL8_xM:&imgrefurl=http://www.acs.psu.edu/drussell/Demos/StandingWaves/StandingWaves.html&docid=rQL8NLCVyxArsM&imgurl=http://www.acs.psu.edu/drussell/Demos/StandingWaves/Opentubeoneend.jpg&w=1600&h=742&ei=VYNZUoyAK4aOigLhvoCABA&zoom=1&ved=1t:3588,r:26,s:0,i:165&iact=rc&page=3&tbnh=153&tbnw=330&start=26&ndsp=16&tx=209&ty=74http://www.google.com/imgres?q=wave+in+pipe&client=safari&rls=en&biw=1039&bih=635&tbm=isch&tbnid=4yOfGhJDUL8_xM:&imgrefurl=http://www.acs.psu.edu/drussell/Demos/StandingWaves/StandingWaves.html&docid=rQL8NLCVyxArsM&imgurl=http://www.acs.psu.edu/drussell/Demos/StandingWaves/Opentubeoneend.jpg&w=1600&h=742&ei=VYNZUoyAK4aOigLhvoCABA&zoom=1&ved=1t:3588,r:26,s:0,i:165&iact=rc&page=3&tbnh=153&tbnw=330&start=26&ndsp=16&tx=209&ty=74http://www.google.com/imgres?q=wave+in+pipe&client=safari&rls=en&biw=1039&bih=635&tbm=isch&tbnid=4yOfGhJDUL8_xM:&imgrefurl=http://www.acs.psu.edu/drussell/Demos/StandingWaves/StandingWaves.html&docid=rQL8NLCVyxArsM&imgurl=http://www.acs.psu.edu/drussell/Demos/StandingWaves/Opentubeoneend.jpg&w=1600&h=742&ei=VYNZUoyAK4aOigLhvoCABA&zoom=1&ved=1t:3588,r:26,s:0,i:165&iact=rc&page=3&tbnh=153&tbnw=330&start=26&ndsp=16&tx=209&ty=74
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The math for pipe wave
s(t, x = 0) = 0∂s
∂x(t, x = L) = 0
xz
y x=0 x=L
s = smax sin(kx) cos(kvt+ φ0)
cos(kL) = 0B.C.@L: kL = (n+1
2)π
k = 2π/λ L = (2n+ 1)λ/4
Tuesday, October 15, 2013
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Math for other cases
Both ends closed: s = smax sin(kx) cos(kvt+ φ)
kL = nπB.C.@L: λ = 2L/n
Both ends open:
kL = nπB.C.@L: λ = 2L/n
s = smax cos(kx) cos(kvt+ φ)
Tuesday, October 15, 2013
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FAQ: Why the sound?
fn = nf1 = nvsound/λ1
λ1 = 2L, n = 1, 2, 3, 4 . . .OO or CC:
λ1 = 4L, n = 1, 3, 5, 7 . . .OC:
From last time, get:
here odd only
Tuesday, October 15, 2013
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Example: singing tube
L (e.g. = 1m)hotair
f1 = v/λ1 = v/2L = 344ms−1/2m = 172Hz.
Tuesday, October 15, 2013
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How does it sound?233Hz = vsound/4L
Tuesday, October 15, 2013
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Interference
s = A1 cos(k(L1 − vt) + φ1) +A2 cos(k(L2 − vt) + φ2)
Superpose two traveling waves..
.Two
sources(speakers)
. sounddetector(your ear)
cos a+ cos b = 2 cos(a− b2
) cos(a+ b
2)use
A1 = A2 φ1 = φ2Let’s keep
it simple, take:
s = 2A cos k(L2 − L1
2) cos(k(
L1 + L22
)− ωt+ φ)get
Constructive: k∆L = 2πnk∆L = (2n+ 1)πDestructive:
∆L = nλ
∆L = (n+1
2)λ
Can be louder or quieter(!) than with just one speaker, depending
on your location. Here’s why:
i.e.i.e.
Tuesday, October 15, 2013
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Beats
A cos(ω1t) +A cos(ω2t) = 2A cos(1
2(ω1 − ω2)t) cos(
1
2(ω1 + ω2)t)
Superpose two sources with different frequencies:
Over time, sometimes addconstructively, sometimesdestructively. Hear beats.
2A cos(1
2(ω1 − ω2)t) modulating wave envelope.
Inside, average frequency.
Tuesday, October 15, 2013
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Doppler effect
You’ve all noticed itwhen a moving siren passes you, frequency goes from high to low.
Police radar speed traps also use Doppler’s
effect. So do bats and dolphins and whales,
with their sonar. Tuesday, October 15, 2013
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Doppler effect Case 1: vsource = 0, vobserver �= 0
Both source and observer see same wavelength, but differing effective speed of sounds, because the observer sees sound’s velocity relative to their own. So they see sound as
moving slower if they’re moving away from it, or faster if they’re moving toward it.
Case 2:
Wavelength is stretched or compressed, depending on whether the source is moving away ortoward the observer. Put these two cases together to get the general case (next slide).
vsource �= 0, vobserver = 0
λemit = vsound/femit = λobs = (vsound − vobserver)/fobs
λobs = λemit − (vsource/femit) = (vsound − vsource)/femit
Tuesday, October 15, 2013
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Doppler, cont. fobserved =
vsound − vobservervsound − vsource
femitted
vsound − vobservervsound − vsource
≈ 1− vobserver − vsourcevsound
vsound � vo, vsif
then
Aside (later), for light: fobs = fsource�
1± vrel/c1∓ vrel/c
Top sign if source is coming at us (blueshift), bottom sign if it’s moving away (red).
Put together:
Signs: replace - signs with +, depending on v directions.
Tuesday, October 15, 2013
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Sonic boom!
sin θ = vsound/vsource
Mach number = vobject/vsound
= 1/Mach number
If >1.
(Concorde, mach 2around 1350 mph!)
Tuesday, October 15, 2013